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In this paper, we extend the source detection in the GOODS-ALMA field (69arcmin$^2$, rms sensitivity $\sigma$ $\simeq$ 0.18 mJy.beam$^{-1}$), to deeperlevels than presented in Franco et al. (2018). Using positional information at3.6 and 4.5 $\mu$m (from Spitzer-IRAC), we explore the presence of galaxiesdetected at 1.1 mm with ALMA below our original blind detection limit of4.8-$\sigma$ at which the number of spurious sources starts to dominate overthat of real sources. In this Supplementary Catalog, we find a total of 16galaxies, including 2 galaxies with no counterpart in HST images (also known asoptically-dark galaxies) down to a 5$\sigma$ limiting depth of H = 28.2 AB(HST/WFC3 F160W). This brings the total sample of GOODS-ALMA 1.1 mm sources to35 galaxies. Galaxies in the new sample cover a wider dynamic range in redshift($z$ = 0.65 - 4.73), are on average twice as large (1.3 vs 0.65 kpc) and andhave lower stellar mass (M$_{\star}^{\rm SC}$ = 7.6$\times$10$^{10}$M$_\odot$vs M$_{\star}^{\rm MC}$ = 1.2$\times$10$^{11}$M$_\odot$). Although exhibitinglarger physical sizes, these galaxies have still far-infrared sizessignificantly more compact than inferred from their optical emission. We showthat the astrometry of the HST image does not only suffer from a globalastrometric shift, as already discussed in previous papers, but also from localshifts. These distortions were artificially introduced in the process ofbuilding the mosaic of the GOODS-South HST image. By comparing the positions ofalmost 400 galaxies detected by HST, Pan-STARRS and ALMA, we create adistortion map which can be used to correct for these astrometric issues.

GOODS-ALMA: Using IRAC and VLA to probe fainter millimeter galaxies